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Lookback time evolution of metals: discarding the closed box model

Published online by Cambridge University Press:  09 March 2010

M. Rodrigues
Affiliation:
GEPI, Observatoire de Paris, CNRS, Universite Paris Diderot, 5 Place Jules Janssen 92190 Meudon, France
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Abstract

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We have gathered a representative sample of 88 intermediate mass galaxies at z~0.6 and have provided robust estimates of their gas phase metallicity based on the strong line method R23. We have found that these galaxies have undergone a strong evolution of their metal content during the last 8 Gyrs. We confirmed the shift about ~0.3dex to lower abundance of the M-Z relation at z~0.6 found by Liang et al. 2006. This result shows that the evolution of the gas phase is still active down to z=0.4 and that the close box model is not a valid scenario for local spiral progenitors.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2010

References

Erb, D. K. et al. 2006, ApJ, 644, 813ECrossRefGoogle Scholar
Lara-Lopez, M. A. et al. 2009, arXiv0907.0450CrossRefGoogle Scholar
Liang, Y.C., Hammer, F., and Flores, H. 2006, A&A, 447, 113LGoogle Scholar
Liu, X. et al. 2008, ApJ, 678, 758LCrossRefGoogle Scholar
Maier, C. et al. 2006, ApJ 639, 858MCrossRefGoogle Scholar
Maiolino, R. et al. 2008, A&A, 488, 463MGoogle Scholar
Puech, M. et al. 2008, A&A, 484, 173PGoogle Scholar
Rodrigues, M et al. 2008, A&A, 492, 371RGoogle Scholar
Shapley, A.E. et al. 2004, ApJ, 612, 108SCrossRefGoogle Scholar
Savaglio, S. et al. 2005, ApJ, 635, 260SCrossRefGoogle Scholar
Tremonti, C., et al. 2004, ApJ 613, 898TCrossRefGoogle Scholar